424 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Peking UniversityCN65 papers
- Kavli Institute for Theoretical SciencesCN31 papers
- Chinese Academy of SciencesCN16 papers
- National Astronomical ObservatoriesCN12 papers
- University of Science and Technology of ChinaCN10 papers
- Institute of High Energy PhysicsCN8 papers
- Centre National de la Recherche ScientifiqueFR7 papers
- Budker Institute of Nuclear PhysicsRU6 papers
- Institute of Modern PhysicsCN6 papers
- Novosibirsk State UniversityRU6 papers
- Ruhr University BochumDE6 papers
- Siberian Branch of the Russian Academy of SciencesRU6 papers
5 papers · 1 filter
Unveiling the solution to the final-parsec problem by combining milli-Hertz gravitational-wave observation and AGN survey
Liang-Gui Zhu, Xian Chen
Massive black hole binaries (MBHBs) could be the loudest gravitational-wave (GW) sources in milli-Hertz (mHz) GW band, but their dynamical evolution may stall when the black holes…
SN2017egm: A Helium-rich Superluminous Supernova with Multiple Bumps in the Light Curves
Jiazheng Zhu, Ning Jiang, Subo Dong +28
When discovered, SN~2017egm was the closest (redshift ) hydrogen-poor superluminous supernova (SLSN-I) and a rare case that exploded in a massive and metal-rich galaxy. Thu…
Long-duration Gamma-ray Burst and Associated Kilonova Emission from Fast-spinning Black Hole--Neutron Star Mergers
Jin-Ping Zhu, Xiangyu Ivy Wang, Hui Sun +5
Here we collect three unique bursts, GRBs\,060614, 211211A and 211227A, all characterized by a long-duration main emission (ME) phase and a rebrightening extended emission (EE) pha…
Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
Chang Liu, Yacheng Kang, Lijing Shao
We investigated the detection rates and early warning parameters of binary neutron star (BNS) populations with decihertz gravitational-wave observatories in a realistic detecting s…
A Comparative Study of Long and Short GRBs. II. A Multi-wavelength Method to distinguish Type II (massive star) and Type I (compact star) GRBs
Ye Li, Bing Zhang, Qiang Yuan
Gamma Ray Burst (GRBs) are empirically classified as long-duration GRBs (LGRBs, 2s) and short-duration GRBs (SGRBs, 2s). Physically they can be grouped into two distinct pr…